Study of the molecular clump associated with the high-energy source HESS J1858+020

Aims. HESS J1858+020 is a weak γ-ray source lying near the southern border of the SNR G35.6-0.4. A molecular cloud, composed of two clumps, shows signs of interaction with both the SNR and a nearby extended HII region. In particular, the southernmost clump coincides with the center of the H.E.S.S. s...

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Detalles Bibliográficos
Autores principales: Paron, S., Giacani, E., Rubio, M., Dubner, G.
Formato: JOUR
Materias:
gamma rays: ISM
ISM: clouds
ISM: individual objects: HESS J1858+020
ISM: supernova remnants
A-density
A-thermal
Angular resolution
Archival data
Atacama
Continuum emission
H II regions
Hadronic interactions
High energy emission
High-energy sources
ISM: individual objects
Molecular clouds
Molecular clumps
Molecular gas
Molecular outflows
Protostars
Shock fronts
Submillimeters
Young stellar objects
Clouds
High energy physics
Stars
Tellurium compounds
Gamma rays
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00046361_v530_n_p_Paron
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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